Cosmology theory compromised

Nature ◽  
1990 ◽  
Vol 346 (6287) ◽  
pp. 800-800 ◽  
Author(s):  
ROBERT L. OLDERSHAW
Keyword(s):  
2014 ◽  
Author(s):  
Mikhail Shaposhnikov
Keyword(s):  

1971 ◽  
Vol 69 (2) ◽  
pp. 295-296 ◽  
Author(s):  
J. Wolfgang Smith

It has often been assumed in cosmology theory(1) that there exists an average density of matter in space which is everywhere greater than zero. Under this assumption the space-time M will be foliated by curves each of which represents the life history of a particle. In keeping with the postulates of general relativity theory we shall refer to these curves as geodesics. Letting X denote the space of particles one obtains a projection f: M → X which assigns to every P ∈ M the particle found at P. Conversely, given the projection f:M → X, one can recover the geodesics: they are precisely the fibres f−1(x), x∈X.


2012 ◽  
Vol 27 (12) ◽  
pp. 1250066 ◽  
Author(s):  
DAMIEN A. EASSON ◽  
PAUL H. FRAMPTON ◽  
GEORGE F. SMOOT

One of the major pillars of modern cosmology theory is a period of accelerating expansion in the early universe. This accelerating expansion, or inflation, must be sustained for at least 30 e-foldings. One mechanism used to drive the acceleration is the addition of a new energy field, called the inflaton; often this is a scalar field. We propose an alternative mechanism which, like our approach to explain the late-time accelerating universe, uses the entropy and temperature intrinsic to information holographically stored on a surface enclosing the observed space. The acceleration is due in both cases to an emergent entropic force, naturally arising from the information storage on the horizon.


Physics Today ◽  
1953 ◽  
Vol 6 (1) ◽  
pp. 17-17
Author(s):  
G. C. McVittie
Keyword(s):  

Pramana ◽  
1999 ◽  
Vol 53 (6) ◽  
pp. 1093-1104 ◽  
Author(s):  
Jayant V Narlikar

2010 ◽  
Vol 60 (1) ◽  
pp. 27-51 ◽  
Author(s):  
Rouzbeh Allahverdi ◽  
Robert Brandenberger ◽  
Francis-Yan Cyr-Racine ◽  
Anupam Mazumdar

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